Title of article :
Near-vertical supersonic and shock-free gas/magma flow at ionian volcanoes: Application to Pillan
Author/Authors :
Cataldo، نويسنده , , Enzo and Davies، نويسنده , , Ashley Gerard and Wilson، نويسنده , , Lionel، نويسنده ,
Issue Information :
روزنامه با شماره پیاپی سال 2013
Pages :
6
From page :
1171
To page :
1176
Abstract :
In 1997, the Pillan volcano on Io was home to a fierce volcanic eruption that emplaced extensive lava flows and a circular plume deposit. The gas/magma flow issuing from the unresolved vent region appeared to form an almost vertical jet. We consider steady eruptions of gas and magma, and take the vent to be either a fissure or a point source. In the fissure scenario, the upper-conduit flow must reach Mach 1 in the 25–75 m depth range to produce the vent velocities of 550–600 m/s that are required to explain the observed plume heights. Conduit wall deflections in the range 20–30° from vertical (values referring to the upper meter of the conduit) and ∼26–30% by mass of incorporated crustal SO2 are also needed. In the point-source scenario, sonic flow conditions and similar velocities are achieved in the depth range 350–500 m for similar conduit wall deflections and gas mass proportions in the erupting mixture. Probably, the source of the 140-km-high plume imaged in 1997 was either a ∼6–11 m-wide fissure, active for ∼14–40 km along strike, or a circular vent ∼125–216 m in diameter, the former scenario being preferred. Finally, a shock-free conduit flow is more likely to sustain a tall lava fountain in a near-vacuum.
Keywords :
IO , volcanism , geological processes , Jupiter , Satellites
Journal title :
Icarus
Serial Year :
2013
Journal title :
Icarus
Record number :
2380103
Link To Document :
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